Dark QCD Origin of the NANOGrav Signal and Self-Interacting Dark Matter
Zihan Wang

TL;DR
This paper proposes a dark QCD-based model that explains the NANOGrav gravitational wave signal and addresses small-scale structure issues via self-interacting dark matter, linking cosmological signals to dark matter properties.
Contribution
It introduces a phenomenological framework with an SU(3)_D gauge theory that accounts for gravitational waves and dark matter self-interactions through a first-order phase transition in the early universe.
Findings
Model fits NANOGrav data comparable to SMBHB predictions.
Dark matter candidate is a 40 GeV dark baryon with self-interactions.
Predicted gravitational wave spectrum has a distinctive shape, testable with future PTAs.
Abstract
The NANOGrav 15-year stochastic gravitational wave background (SGWB) amplitude lies at the upper edge of population synthesis predictions for supermassive black hole binaries (SMBHBs), motivating exploration of additional cosmological sources. We present a phenomenological framework based on an gauge theory that can simultaneously accommodate the gravitational wave signal and resolve small-scale structure anomalies via Self-Interacting Dark Matter (SIDM). The dark matter candidate is a heavy dark baryon with mass ~GeV, which self-interacts through a light pseudo-dilaton --~MeV as a pseudo-Goldstone boson of approximate scale invariance arising in near-conformal gauge theories with -- light flavors. A first-order phase transition at the MeV scale, enabled by…
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